The problem of the pulsation of the Cepheid CO Aurigae.

Details The problem of the pulsation of the Cepheid CO Aurigae. The problem of the pulsation of the Cepheid CO Aurigae.

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...309..144a&link_type=abstract

Astronomy and Astrophysics, v.309, p.144-146

Astronomy and Astrophysics

Astrophysics

3

Stars: Individual: Co Aur, Cepheids, Stars: Oscillations

Scientific paper

CO Aur is unique among the double mode Cepheids in the Galaxy owing to its period ratio 0.80, and it should be pulsating in the first and second overtone mode. With the new opacities it is not possible to obtain a satisfactory pulsation model for CO Aur which is also compatible with the models of the other beat, bump and first overtone Cepheids. While the other Cepheid models require a low mass for a given luminosity, the CO Aur model requires mass and luminosity which are compatible with standard values.

Affiliated with

Also associated with

No associations

Rating

The problem of the pulsation of the Cepheid CO Aurigae. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The problem of the pulsation of the Cepheid CO Aurigae., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The problem of the pulsation of the Cepheid CO Aurigae. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1351105